Light Curves of Short GRB Pulses

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We provide a method to estimate the energy-flux light-curve of gamma-ray bursts with high time-resolution by applying averaged, bolometric corrections to the count light-curves. This gives the possibility to study light curves of short pulses in energy flux instead of count rates. We found that in most cases a correction is not necessary, but for a few cases it is important. We illustrate this with three pulses from BATSE bursts, for two of which a correction is necessary.

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